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Tenenbaum, R. Brahm, R. P. Butler, R. Vanderspek, S. Durkan, S. Quinn, S. Seager, S. Shectman, Th. Henning, V. Suc, W. Bhatti, Z. Csubry","submitted_at":"2018-12-21T23:13:24Z","abstract_excerpt":"We report the discovery of HATS-71b, a transiting gas giant planet on a P = 3.7955 day orbit around a G = 15.35 mag M3 dwarf star. HATS-71 is the coolest M dwarf star known to host a hot Jupiter. The loss of light during transits is 4.7%, more than any other confirmed transiting planet system. The planet was identified as a candidate by the ground-based HATSouth transit survey. It was confirmed using ground-based photometry, spectroscopy, and imaging, as well as space-based photometry from the NASA TESS mission (TIC 234523599). 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